Aims and Scope of Astronomy Reports
Astronomy Reports (Russian: ÐÑтрономичеÑкий журнал, Astronomicheskii Zhurnal), is a Russian, monthly, peer reviewed, scientific journal. This journal tends to focus its publishing efforts on original research regarding astronomical topics. Other types of reporting are also included such as chronicles, proceedings of international conferences, and book reviews. Founded in 1924, it is described as the most prominent astronomy journal during the age of the Soviet Union. Originally a print version, it is also available online. The Editor-in-Chief was Alexander A. Boyarchuk, Institute of Astronomy of the Russian Academy of Sciences, Moscow, Russia. Less
Key Metrics
CiteScore 

1.8
H-Index 

33
Impact Factor 

< 5
SJR 

Q3Astronomy and Astrophysics

SNIP 

0.57
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Topics Covered on Astronomy Reports
Astronomy Reports Journal Specifications
| Overview | |
| Publisher | PLEIADES PUBLISHING INC |
| Language | English |
| Frequency | Monthly |
| General Details |
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Recently Published Papers in Astronomy Reports
Using Plasma Jet Sources Based on Compact Coaxial Accelerators for Laboratory Modeling of Pulsed Astrophysical Phenomena in a Large Plasma Chamber
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Simulation of Transverse Collisionless Jets in Laser Plasma Experiments
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X-Ray Spectral Diagnostics of the Interaction Region of a Supersonic Plasma Flow with a Gas Wall in Laboratory Experiments with Astrophysical Similarity
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Using Plasma Jet Sources Based on Compact Coaxial Accelerators for Laboratory Modeling of Pulsed Astrophysical Phenomena in a Large Plasma Chamber
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MHD Simulations of Magnetized Rotating Jets
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Numerical Modeling of the Generation and Dynamics of Plasma Flows at Plasma Focus Type Installations Within the Framework of Laboratory Modeling of Jets from Young Stellar Objects
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On the Possibility of Eliminating the Time Parallax Effect in Registration of Moving Objects on CMOS Matrices in Rolling Shutter Mode
- 1 Dec 2025
- Astronomy Reports
X-Ray Spectral Diagnostics of the Interaction Region of a Supersonic Plasma Flow with a Gas Wall in Laboratory Experiments with Astrophysical Similarity
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